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GCN Circular 1853

Subject
IPN triangulation of GRB030202 (annulus)
Date
2003-02-04T16:39:12Z (22 years ago)
From
Kevin Hurley at UCBerkeley/SSL <khurley@sunspot.ssl.berkeley.edu>
K. Hurley and T. Cline, on behalf of the Ulysses GRB team, and

A. von Kienlin, G. Lichti, and A. Rau, on behalf of the
INTEGRAL SPI-ACS GRB team, report:

Ulysses and INTEGRAL (SPI-ACS) observed this burst at 62460 s.
As observed by Ulysses, it had a duration of approximately  15
seconds, a 25-100 keV fluence of approximately  7.9E-07 erg/cm2, and a
peak flux of approximately  3.2E-07 erg/cm2 s over 0.50 seconds.

We have triangulated it to a preliminary annulus centered at
RA, Decl. (2000) = 356.094, -40.659 degrees, with radius
26.688 +/- 0.217 degrees (3 sigma).

This annulus can be refined and/or constrained, but as this
burst was not observed by Mars Odyssey, a small error box
cannot be obtained for it.
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